SPH simulations of tidally unstable accretion discs in cataclysmic variables

Monthly Notices of the Royal Astronomical Society

Volumn 279, Issue 2, 1996, Pages 402-414

  Murray, J R ^a  

^a UNIVERSITY OF TORONTO   (Canada)

Author keywords

Accretion, accretion discs; Binaries: close; Hydrodynamics; Instabilities; Methods: numerical; Novae, cataclysmic variables

Indexed keywords

ENERGY DISSIPATION; MASS TRANSFER; NUMERICAL METHODS; ORBITS;

ACCRETION DISCS; ACCRETION: ACCRETION DISKS; BINARIES: CLOSE; CATACLYSMIC VARIABLES; DISK MODEL; METHOD: NUMERICAL; NOVAE CATACLYSMIC VARIABLES; SPH CODE; SPH SIMULATION; TWO-DIMENSIONAL;

HYDRODYNAMICS;

EID: 0001185899     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/279.2.402     Document Type: Article

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